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Fig. 5
Best-fit analytic models on MIR SEDs of the SNe. The 3.6 μm and sometimes the 4.5 μm fluxes are usually not included in the fitting (see text). The fittings that contain hot and warm components for SN 2004A and SN 2006my are shown in Fig. 6.
This figure is made of several images, please see below:
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